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Home > Art, Film & Photography > Astronomia y Astrofisica: Estrella, Radioastronomia, Brote de Rayos Gamma, Sistema de Datos Astrofisicos, Metrica de Alcubierre
Astronomia y Astrofisica: Estrella, Radioastronomia, Brote de Rayos Gamma, Sistema de Datos Astrofisicos, Metrica de Alcubierre

Astronomia y Astrofisica: Estrella, Radioastronomia, Brote de Rayos Gamma, Sistema de Datos Astrofisicos, Metrica de Alcubierre


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About the Book

Fuente: Wikipedia. Paginas: 31. Capitulos: Estrella, Radioastronomia, Brote de rayos gamma, Sistema de Datos Astrofisicos, Metrica de Alcubierre, Union Astronomica Internacional, Radiacion cosmica, Disco de acrecimiento, Onda gravitacional, Ano Internacional de la Astronomia, George Ellis, Lente gravitacional, Tubo de Krasnikov, Efecto Shapiro, LIGO, Radiofuente, Implosion, Nanodiamante, Letra de Bayer. Extracto: Los brotes de rayos gamma (tambien conocidos como GRB en sus siglas en ingles, BRG en espanol) son destellos de rayos gamma asociados con explosiones extremadamente energeticas en galaxias distantes. Son los eventos electromagneticos mas luminosos que ocurren en el universo. Los brotes pueden durar desde unos nanosegundos hasta cerca de una hora, pero por lo general, un brote tipico suele durar unos pocos segundos. Con frecuencia son seguidos por una luminiscencia residual de larga duracion de radiacion a longitudes de onda mayor, (rayos X, radiacion ultravioleta, luz visible, radiacion infrarroja y radiofrecuencia). Se cree que muchos de los BRG son haces muy colimados con radiacion intensa producidos a causa de una supernova, cuando una estrella de rapida rotacion y gran masa colapsa para formar un agujero negro. Una subclase de BRG (denominados brotes -cortos-) parecen ser originados por un proceso diferente, posiblemente la fusion de estrellas binarias de neutrones; mientras que los -brotes largos- parecen derivarse a causa de la muerte de estrellas masivas; es decir, por una supernova, o incluso, por una hipernova. Los dos tipos de brotes se diferencian por su tiempo de duracion: los primeros suelen durar menos de dos segundos, mientras que los otros, tienden a alargarse durante mas tiempo. Las fuentes de los BRG se encuentran a miles de millones de anos luz de distancia de la Tierra, lo que implica que las explosiones son extremadamente energeticas (se ha comprobado que un brote tipico puede generar la misma energia que el sol en un periodo de die...


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Product Details
  • ISBN-13: 9781231355091
  • Publisher: Books LLC
  • Publisher Imprint: Books LLC
  • Height: 246 mm
  • No of Pages: 32
  • Spine Width: 2 mm
  • Weight: 77 gr
  • ISBN-10: 1231355093
  • Publisher Date: 25 May 2011
  • Binding: Paperback
  • Language: Spanish
  • Returnable: N
  • Sub Title: Estrella, Radioastronomia, Brote de Rayos Gamma, Sistema de Datos Astrofisicos, Metrica de Alcubierre
  • Width: 189 mm


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